Central Bureau for Astronomical Telegrams

Central Bureau for Astronomical Telegrams -- Image credits

IAUC 4397: N Sgr 1987; U Sco; 1987A; 1986l

The following International Astronomical Union Circular may be linked-to from your own Web pages, but must not otherwise be redistributed (see these notes on the conditions under which circulars are made available on our WWW site).


Read IAUC 4396  SEARCH Read IAUC 4398
IAUC number


                                                  Circular No. 4397
Central Bureau for Astronomical Telegrams
INTERNATIONAL ASTRONOMICAL UNION
Postal Address: Central Bureau for Astronomical Telegrams
Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A.
TWX 710-320-6842 ASTROGRAM CAM    Telephone 617-495-7244/7440/7444


NOVA SAGITTARII 1987
     R. H. McNaught, Siding Spring Observatory, reports his discovery
of a nova on 85-mm patrol camera Tri-X films, and he provides
the following magnitude estimates:  May 11.80 UT, [11.5; 18.79,
10.5; 20.48, 10; 21.68, 10.5; 24.39, 10 (visual); 25.4, 10 (visual).
No pre-nova candidate is visible on ESO B film nor on U.K.
Schmidt J, I, or R survey films.  McNaught provides his measurement
of the nova's position from a plate taken with the Uppsala Southern
Schmidt telescope:  R.A. = 17h56m28.96, Decl. = -32 16'13.4 (+/- 0".4,
equinox 1950.0).  An IPCS spectrum taken by S. Lee, B. Peterson, and T.
Shanks with the Anglo-Australian Telescope on May 24 shows the star
to be red with strong H-alpha emission (FWHM about 1000 km/s).


U SCORPII
     Visual magnitude estimates:  May 21.65 UT, 12.3 (S. Sakuma,
Kawasaki, Japan); 22.65, 13.4 (McNaught); 23.45, 14.0 (T. Cragg,
Siding Spring Observatory); 25.66, 14.2 (McNaught).


SUPERNOVA 1987A IN THE LARGE MAGELLANIC CLOUD
     R. J. Patterson and P. A. Ianna, Astronomy Department, University
of Virginia, report:  "We have measured, using the Mt. Stromlo
PDS microdensitometer, the position of SN 1987A from 4 plates (
IIaO, scale 18".85/mm) taken on 1987 Feb. 25 with the 0.66-m Yale-
Columbia refractor located at Mt. Stromlo; two of the plates were
taken with a neutral-density filter which reduced the intensity of
the SN by about 4.5 mag.  Using 19 transfer stars measured with 9 Perth
standard stars, we find the following position for the SN:  R.A. =
5h35m49.896 +/- 0".16, Decl. = -69 17'58.26 +/- 0".05, equinox 1950.0."
     Visual magnitude estimates:  May 21.57 UT, 2.8 (McNaught);
22.33, 2.8 (D. A. J. Seargent, The Entrance, N.S.W.); 23.44, 2.9
(G. Garradd, Tamworth, N.S.W.); 24.56, 2.8 (McNaught); 25.36, 2.8
(Seargent); 25.40, 2.9 (McNaught).


COMET WILSON (1986l)
     Total visual magnitude estimates (cf. IAUC 4391):  May 17.13
UT, 6.2 (A. Hale, Las Cruces, NM, 10x50 binoculars); 19.42, 6.2
(Garradd, 7x50 binoculars); 20.42, 6.3 (Garradd); 21.40, 6.3
(Garradd); 23.42, 6.3 (Garradd); 24.43, 6.5 (Garradd).


1987 May 25                    (4397)            Daniel W. E. Green

Read IAUC 4396  SEARCH Read IAUC 4398


Our Web policy. Index to the CBAT/MPC/ICQ pages.


Valid HTML 4.01!